Magnetic field generation in plasma waves driven by co-propagating intense twisted lasers

ORAL

Abstract

We present a new magnetic field generation mechanism in underdense plasmas driven by the beating of two, co-propagating, Laguerre-Gaussian (LG) orbital angular momentum (OAM) laser pulses with different frequencies and also different twist indices. Results of 3D particle-in-cell simulations show that the twisted ponderomotive force drives up an electron plasma wave with a helical rotating structure. For the case of 300 fs duration, 3.8×1017 W/cm2 peak laser intensity we observe magnetic field of up to 0.4 MG. We will also outline a theoretical model, based on cold electron fluid equations, that reproduces that pertinent features of the PIC simulations – including the axial magnetic field – in the appropriate limits and elucidates the mechanism and highlights its scaling with key parameters.To second order, there is a nonlinear rotating current leading to the onset of an intense, static axial magnetic field, which persists over a long time in the plasma (ps scale) after the laser pulses have passed by. Applications of this new method of magnetic field creation will be discussed.

*This work is supported by the Royal Society.

Presenters

  • Yin Shi

    • UC San Diego , Imperial College London

Authors

  • Yin Shi

    • UC San Diego , Imperial College London
  • Jorge M Vieira

    • ISCTE - Inst Universitario Lisboa
    • Instituto Superior Técnico, Lisbon, Portugal
    • GoLP/Instituto Superior Tecnico
    • Inst Superior Tecnico (IST)
    • GoLP/IPFN Instituto Superior Técnico, Universidade de Lisboa, Lisboa, Portugal
    • Instituto de Plasmas e Fusão Nuclear-Laboratório Associado
    • Inst Superior Tecnico (IST), Inst Superior Tecnico (IST)
  • Raoul M Trines

    • Rutherford Appleton Lab
  • Robert Bingham

    • Rutherford Appleton Lab
    • Rutherford Appleton Lab, University of Strathclyde
    • Rutherford Appleton Lab, Univeristy of Stratchclyde
  • Baifei Shen

    • Shanghai Inst of Opt & Fine Mechanics
  • Robert J Kingham

    • Imperial College London